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- Brightness Variations in Saturn's Satellite 1995S5
-
- This sequence of 100 sec exposures taken with HST's Wide Field and
- Planetary Camera (WFPC2) in planetary mode on 10 August 1995 shows the
- newly discovered object 1995S5 (red arrows) moving in its orbit around
- the planet. As it moves further from Saturn, its brightness decreases
- appreciably. This brightness variation is more consistent with that
- expected for an elongated, opaque clump of ring material than for a
- satellite, leading to the suspicion that 1995S5 is in fact a ring arc
- rather than a previously undiscovered satellite. It is likely that it
- lies within the narrow, braided F Ring.
-
- In addition to 1995S5, the larger satellites Mimas and Epimetheus are
- visible in each frame. Mimas is the bright object below the rings,
- and is seen partly shadowed by the rings in the first frame. In
- subsequent frames it is in full sunlight. Epimetheus is near the
- eastern ansa of the rings, moving slowly outward. In the last frame of
- the sequence tiny Pandora has emerged from Saturn's shadow about 2
- arcsec from the planet's limb.
-
- These images were obtained one to two hours before the Earth crossed
- Saturn's ring plane and an 8922 A methane band filter was used to
- reduce the scattered light from the planet. An average of several
- other frames has been subtracted from each image to remove the light
- from the edge-on rings, and so reveal any faint satellites.
-
- Credit: Phil Nicholson (Cornell University), Mark Showalter
- (NASA-Ames/Stanford) and NASA
-